Browsing by Author Wood, P R

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Issue DateTitleAuthor(s)Citation
2006Comparison of dynamical model atmospheres of Mira variables with mid-infrared interferometric and spectroscopic observationsScholz, M; Ohnaka, K; Wood, P R; PhysicsComparison of dynamical model atmospheres of Mira variables with mid-infrared interferometric and spectroscopic observations, Astronomy & Astrophysics, vol.446,(3),2006,pp 1119-1127
2011Dynamical opacity-sampling models of Mira variables - II. Time-dependent atmospheric structure and observable properties of four M-type model seriesIreland, Michael; Scholz, Michael; Wood, P R; Physics; PhysicsDynamical opacity-sampling models of Mira variables - II. Time-dependent atmospheric structure and observable properties of four M-type model series, Monthly Notices of the Royal Astronomical Society, vol.418, 1, 2011,pp 114-128
2008Dynamical opacity-sampling models of Mira variables – I. Modelling description and analysis of approximationsIreland, Michael; Scholz, Michael; Wood, P R; Physics; PhysicsDynamical opacity-sampling models of Mira variables – I. Modelling description and analysis of approximations, Monthly Notices Royal Astronomical Society, vol.391, N/A, 2008,pp 1994-2002
2011Inhomogeneities in molecular layers of Mira atmospheresScholz, Michael; Boboltz, D A; Ireland, M.; Karovicova, I; Ohnaka, K; Van Wyk, F; Whitelock, P. A.; Wittkowski, M; Wood, P R; Zijlstra, Albert A.; PhysicsInhomogeneities in molecular layers of Mira atmospheres, Astronomy and Astrophysics (A and A), vol.532, N/A, 2011,pp L7-1-5
2005The K-band intensity profile of R Leonis probed by VLTI/VINCIScholz, M; Ciroi, S; Fedele, D; Paresce, F.; Wittkowski, M; Wood, P R; PhysicsThe K-band intensity profile of R Leonis probed by VLTI/VINCI, Astronomy & Astrophysics, vol.431,(3),2005,pp 1019-1026
2004On The Observability Of Geometric Pulsation Of M-Type Mira VariablesIreland, Michael; Scholz, Michael; Wood, P R; Physics; PhysicsOn The Observability Of Geometric Pulsation Of M-Type Mira Variables, Monthly Notices of the Royal Astronomical Society, vol.352,(1),2004,pp 318-324
2003Optical and near-IR spectra of O-rich Mira variables: A comparison between models and observationsScholz, Michael; Lancon, A; Tej, A; Wood, P R; PhysicsOptical and near-IR spectra of O-rich Mira variables: A comparison between models and observations, Astronomy & Astrophysics, vol.412,(2),2003,pp 481-494
2015What causes the large extensions of red supergiant atmospheres? Comparisons of interferometric observations with 1D hydrostatic, 3D convection, and 1D pulsating model atmospheresScholz, Michael; Abellan, F; Arroyo-Torres, B; Chiavassa, A; Freytag, B; Hauschildt, P; Marcaide, J; Wittkowski, M; Wood, P R; PhysicsWhat causes the large extensions of red supergiant atmospheres? Comparisons of interferometric observations with 1D hydrostatic, 3D convection, and 1D pulsating model atmospheres, Astronomy and Astrophysics, vol.575, N/A, 2015,pp 1-17